Total electric charge on the earth,

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SUMMARY

The total electric charge on Earth can be calculated using the volume density of charge, represented as ρ = ρs * r / R, where ρs is the surface density and R is the Earth's radius. The total charge is proven to be Q = πρsR³. Gauss's law is applied to derive the electric field E outside the Earth (r > R) and within its interior (r < R). The discussion also covers the calculation of the divergence of E, denoted as ∇·E, and emphasizes the correct integration method to eliminate constants in the final expressions.

PREREQUISITES
  • Understanding of Gauss's Law in electrostatics
  • Familiarity with spherical coordinates and volume integrals
  • Knowledge of electric field concepts and charge density
  • Basic calculus, particularly integration techniques
NEXT STEPS
  • Study the application of Gauss's Law in different geometries
  • Learn about electric field calculations for non-uniform charge distributions
  • Explore advanced integration techniques in spherical coordinates
  • Investigate the implications of charge density variations in electrostatics
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Students in physics, particularly those studying electromagnetism, educators teaching electrostatics, and researchers interested in charge distribution models.

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Homework Statement


The Earth can be regarded as a sphere of radius R,
the volume density of charge distributed as [tex]\rho = \frac{\rho_s r}{R}[/tex]
where the density is 0 at thcce centre and rises linearly with radius until it reaches ps at the Earth's surface

i) prove that the total charge on the Earth is [tex]\pi \rho_s R^3[/tex]

ii) use gauss's law to find an expression for E at the point r outside the Earth (r>R)

iii) use gauss's law to find an expression for E within the Earth's interior (r<R)

iv) write expressions for the x-, y- and z- components of E at a point outside the Earth and calculate [tex]\bf{\nabla .E }<br /> <br /> <h2>Homework Equations</h2><br /> <br /> Qenclosed = [tex]\int_v \rho d\tau.[/tex] (for a volume)<br /> <br /> [tex]\oint_S \bf{E} . d\bf{a} = \frac{1}{\epsilon} Qenclosed[/tex]<br /> <br /> <h2>The Attempt at a Solution</h2><br /> <br /> [tex]\int_v \rho \dtau[/tex]<br /> <br /> substituting in the given rho,<br /> <br /> [tex]\int \rho_s \frac{r}{R} \dtau[/tex]<br /> <br /> the outer radius r is = R so it just becomes R/R =1,<br /> <br /> [tex]\rho_s *1 \int \dtau[/tex]<br /> <br /> this is where I integrate the dtau and it should give me the volume of a sphere<br /> <br /> [tex]\rho_s \frac{4}{3}\pi r^3[/tex]<br /> <br /> this sort of looks like the answer I'm looking for <br /> HOWEVER I DONT KNOW HOW TO GET RID OF THE 4/3 constant!<br /> what have I done wrong?<br /> i've tried heaps of other methods, but I'm always getting some type of constant out the front[/tex]
 
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The density is proportional to r, as you wrote, but you can't pull this factor of r outside the integral. You should write:
[tex]\int_0^R\rho(r)d\tau = \int_0^R\rho_s\frac{r}{R}4\pi r^2 dr = 4\pi\frac{\rho_s}{R}\int_0^Rr^3 dr = 4\pi \frac{\rho_s}{R} \frac{R^4}{4} = \pi\rho_sR^3[/tex]

Does this make sense?
 
phyzguy said:
The density is proportional to r, as you wrote, but you can't pull this factor of r outside the integral. You should write:
[tex]\int_0^R\rho(r)d\tau = \int_0^R\rho_s\frac{r}{R}4\pi r^2 dr = 4\pi\frac{\rho_s}{R}\int_0^Rr^3 dr = 4\pi \frac{\rho_s}{R} \frac{R^4}{4} = \pi\rho_sR^3[/tex]

Does this make sense?

Yes thanks, I actually ended up doing it like this myself last night, I just didn't update it here on PF
 

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